Seismic constraints on the radial dependence of the internal rotation profiles of six Kepler subgiants and young red giants

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Table 2

Characteristics of the fit performed by each fitting group to extract the mode frequencies and rotational splittings from the power spectra.

Fitter	Method	Stars fitted	Final fit

Appourchaux	MLE Global^a	A → F	–
Benomar	MCMC^b	D, F	D, F
Campante	MLE Global^a	E	–
Davies	MLE Global^a	A → F	–
Deheuvels	MLE Global^a	A → F	A, B, C, E
	MLE Local^c	A → F	–
Regulo	MLE Global^a	A → F	–
Stahn	MLE Local^c	A → F	–

Notes. The first column provides the name of the fitter. The second column gives the method followed by the fitter. The third column lists the stars that were fitted. The fourth column lists the stars for which the fitter performed the final fit.

Reference.

^(a)

Appourchaux et al. (2008);

^(b)

Benomar et al. (2009);

^(c)

Anderson et al. (1990).

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